Physics
Scientific paper
Sep 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983apjs...53...93g&link_type=abstract
Astrophysical Journal Supplement Series (ISSN 0067-0049), vol. 53, Sept. 1983, p. 93-103. Research supported by the Natural Scie
Physics
26
Equations Of State, Neutron Stars, Radial Distribution, Stellar Oscillations, Vibration Mode, Density Distribution, Frequencies, Matter (Physics), Nuclear Quadrupole Resonance, Pulsars
Scientific paper
The investigation of the influence of the equation of state of matter (in the nuclear density regime) on the dynamical behavior of neutron stars is continued. The properties of the two lowest frequency radial oscillation modes of neutron stars, constructed from 13 equations of state, are presented. It is found that the frequencies of both radial oscillation modes studied here are generally higher than the frequency of the corresponding quadrupole f-mode.
Glass Edward N.
Lindblom Lee
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